Properties of magnetohydrodynamic turbulence in the solar wind as observed by Ulysses at high heliographic latitudes

Geophysical Research Letters

Volumn 22, Issue 23, 1995, Pages 3393-3396

  Goldstein, B E ^a   Smith, E J ^a   Balogh, A ^b   Horbury, T S ^b   Goldstein, M L ^c   Roberts, D A ^c  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b IMPERIAL COLLEGE LONDON   (United Kingdom)

^c NASA GODDARD SPACE FLIGHT CENTER   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 84989593231     PISSN: 00948276     EISSN: 19448007     Source Type: Journal    
DOI: 10.1029/95GL03183     Document Type: Article

References (31)

1. Large‐scale solar wind fluctuations in the inner heliosphere at low solar activity
2. Statistical properties of MHD fluctuations associated with high‐speed streams from Helios‐2 observations
3. Large‐amplitude Alfvén waves in the interplanetary medium, 2
4. Radial variations of large‐scale magnetohydrodynamic fluctuations
5. The hydromagnetic equations
6. Hydromagnetic dynamo theory
7. High beta turbulence in two‐dimensional magnetohydrodynamics
8. Power spectral signatures of interplanetary corotating and transient flows
9. Magnetohydrodynamic turbulence in the solar wind
10. Alfvén waves, alpha particles, and pickup ions in the solar wind
11. Non‐WKB Alfvén waves in the solar wind
12. Magnetic field signatures of unevolved turbulence in solar polar flows
13. Ulysses magnetic field observations of fluctuations within polar coronal flows
14. Observations of evolving turbulence in the polar solar wind
15. The polar heliospheric magnetic field
16. Interpretation and consequences of large‐scale magnetic variances observed at high heliographic latitude
17. Inertial range of hydromagnetic turbulence
18. Measurement of the rugged invariants of magnetohydrodynamic turbulence
19. Stationarity of magnetohydrodynamic fluctuations in the solar wind
20. Turbulent polar heliospheric fields
21. MHD simulation of the radial evolution and stream structure of solar wind turbulence
22. The amplitudes of interplanetary fluctuations: Stream structure, heliocentric distance, and frequency dependence
23. Origin and evolution of fluctuations in the solar wind: Helios observations and Helios‐Voyager comparisons
24. The nature and evolution of magnetohydrodynamic fluctuations in the solar wind: Voyager observations
25. Velocity shear generation of solar wind turbulence
26. Solar wind speed structure in the inner corona at 3–12 Rs
27. Latitudinal variation of speed and mass flux in the acceleration region of the solar wind inferred from spectral broadening measurements